UBV photometry of V616 MON /A0620-00/

Details UBV photometry of V616 MON /A0620-00/ UBV photometry of V616 MON /A0620-00/

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....81..368c&link_type=abstract

Astronomy and Astrophysics, vol. 81, no. 3, Jan. 1980, p. 368-370. Research supported by the Universite Paris VII, Conselho Nac

Astronomy and Astrophysics

Astronomy

2

Novae, Stellar Spectrophotometry, Ubv Spectra, Variable Stars, X Ray Sources, Eclipses, Electrophotometry, Sas-3, Satellite Observation, Spaceborne Astronomy, Stellar Occultation, X Ray Astronomy, X Ray Spectra

Scientific paper

Photoelectric photometry of V616 Mon (A0620-00) obtained in October 1975 and March 1976 shows evidence of a low amplitude intensity modulation with an 8-10 day time scale. This modulation may be related to that detected in X-rays in January 1976. Its amplitude increased with wavelength in March but no such effect was detectable in October. An eclipse-like feature appears superposed onto one cycle of the modulation in March. Significant intra-night variability was observed in October.

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